Regolith stratigraphy at the Chang'E-3 landing site as seen by lunar penetrating radar

The Chang'E‐3 lunar penetrating radar (LPR) observations at 500 MHz reveal four major stratigraphic zones from the surface to a depth of ~20 m along the survey line: a layered reworked zone (

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Veröffentlicht in:Geophysical research letters 2015-12, Vol.42 (23), p.10,179-10,187
Hauptverfasser: Fa, Wenzhe, Zhu, Meng-Hua, Liu, Tiantian, Plescia, Jeffrey B.
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container_end_page 10,187
container_issue 23
container_start_page 10,179
container_title Geophysical research letters
container_volume 42
creator Fa, Wenzhe
Zhu, Meng-Hua
Liu, Tiantian
Plescia, Jeffrey B.
description The Chang'E‐3 lunar penetrating radar (LPR) observations at 500 MHz reveal four major stratigraphic zones from the surface to a depth of ~20 m along the survey line: a layered reworked zone (
doi_str_mv 10.1002/2015GL066537
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The reworked zone has two to five distinct layers and consists of surface regolith. The paleoregolith buried by the ejecta from a 500 m crater is relatively homogenous and contains only a few rocks. Population of buried rocks increases with depth to ~2 m at first, and then decreases with depth, representing a balance between initial deposition of the ejecta and later turnover of the regolith. Combining with the surface age, the LPR observations indicate a mean accumulation rate of about 5–10 m/Gyr for the surface regolith, which is at least 4–8 times larger than previous estimation. Key Points Chang'E‐3 high‐frequency lunar penetrating radar observations are presented Four major stratigraphic zones at the Chang'E‐3 landing site are observed Regolith accumulation rate is at least 4–8 times higher than previous estimation</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1002/2015GL066537</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Accumulation ; Age ; Basalt ; Chinese spacecraft ; Craters ; Deposition ; Depth ; Ejecta ; Ejection ; Landing sites ; Lunar exploration ; Lunar landing ; lunar penetrating radar ; paleoregolith ; Radar ; Regolith ; regolith thickness ; Rock ; Rocks ; Stratigraphy ; Surveying</subject><ispartof>Geophysical research letters, 2015-12, Vol.42 (23), p.10,179-10,187</ispartof><rights>2015. American Geophysical Union. 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Res. Lett</addtitle><description>The Chang'E‐3 lunar penetrating radar (LPR) observations at 500 MHz reveal four major stratigraphic zones from the surface to a depth of ~20 m along the survey line: a layered reworked zone (&lt;1 m), an ejecta layer (~2–6 m), a paleoregolith layer (~4–11 m), and the underlying mare basalts. The reworked zone has two to five distinct layers and consists of surface regolith. The paleoregolith buried by the ejecta from a 500 m crater is relatively homogenous and contains only a few rocks. Population of buried rocks increases with depth to ~2 m at first, and then decreases with depth, representing a balance between initial deposition of the ejecta and later turnover of the regolith. Combining with the surface age, the LPR observations indicate a mean accumulation rate of about 5–10 m/Gyr for the surface regolith, which is at least 4–8 times larger than previous estimation. Key Points Chang'E‐3 high‐frequency lunar penetrating radar observations are presented Four major stratigraphic zones at the Chang'E‐3 landing site are observed Regolith accumulation rate is at least 4–8 times higher than previous estimation</description><subject>Accumulation</subject><subject>Age</subject><subject>Basalt</subject><subject>Chinese spacecraft</subject><subject>Craters</subject><subject>Deposition</subject><subject>Depth</subject><subject>Ejecta</subject><subject>Ejection</subject><subject>Landing sites</subject><subject>Lunar exploration</subject><subject>Lunar landing</subject><subject>lunar penetrating radar</subject><subject>paleoregolith</subject><subject>Radar</subject><subject>Regolith</subject><subject>regolith thickness</subject><subject>Rock</subject><subject>Rocks</subject><subject>Stratigraphy</subject><subject>Surveying</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqFkctOwzAQRS0EEuWx4wMssYAFgXGc2PESKihIpTzEQ2JjTZNpGwhJsVNB_x5DEUIsYDMzi3NHM_cytiVgXwDEBzGItNcHpVKpl1hHmCSJMgC9zDoAJsyxVqtszftHAJAgRYfdXdO4qcp2wn3rsC3HDqeTOceWtxPi3QnW453jSPIK66Ksx9yXLXH03BPVfDjn1axGx6dU06c8EA4LdBtsZYSVp82vvs5uT45vuqdR_6J31j3sR5gmsYjyYWoUKQUqBdKFwaGGLCMtUZGIsyRTuii0ygGpQGVCLTThSAmRy1FuhFxnu4u9U9e8zMi39rn0OVXhXGpm3orwfhqsAfU_qnUwLsmMCej2L_Sxmbk6PGKFEZApqXXyJ6VDAolUkAVqb0HlrvHe0chOXfmMbm4F2I_U7M_UAh4v8NeyovmfrO1d90OLP1yIFqLSt_T2LUL3ZJWWOrX3g559GJwP7q8uwR7Jd7DupOo</recordid><startdate>20151216</startdate><enddate>20151216</enddate><creator>Fa, Wenzhe</creator><creator>Zhu, Meng-Hua</creator><creator>Liu, Tiantian</creator><creator>Plescia, Jeffrey B.</creator><general>Blackwell Publishing Ltd</general><general>John Wiley &amp; Sons, Inc</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>8FD</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>KL.</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope><scope>7UA</scope><scope>C1K</scope></search><sort><creationdate>20151216</creationdate><title>Regolith stratigraphy at the Chang'E-3 landing site as seen by lunar penetrating radar</title><author>Fa, Wenzhe ; Zhu, Meng-Hua ; Liu, Tiantian ; Plescia, Jeffrey B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a5421-cb596e660650e7d9ab7088e73a6e1284867dd76c0aeda69aedd7eaf611c3fc913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Accumulation</topic><topic>Age</topic><topic>Basalt</topic><topic>Chinese spacecraft</topic><topic>Craters</topic><topic>Deposition</topic><topic>Depth</topic><topic>Ejecta</topic><topic>Ejection</topic><topic>Landing sites</topic><topic>Lunar exploration</topic><topic>Lunar landing</topic><topic>lunar penetrating radar</topic><topic>paleoregolith</topic><topic>Radar</topic><topic>Regolith</topic><topic>regolith thickness</topic><topic>Rock</topic><topic>Rocks</topic><topic>Stratigraphy</topic><topic>Surveying</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Fa, Wenzhe</creatorcontrib><creatorcontrib>Zhu, Meng-Hua</creatorcontrib><creatorcontrib>Liu, Tiantian</creatorcontrib><creatorcontrib>Plescia, Jeffrey B.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>Technology Research Database</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science &amp; Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy &amp; Non-Living Resources</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science &amp; Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Water Resources Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Fa, Wenzhe</au><au>Zhu, Meng-Hua</au><au>Liu, Tiantian</au><au>Plescia, Jeffrey B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Regolith stratigraphy at the Chang'E-3 landing site as seen by lunar penetrating radar</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>2015-12-16</date><risdate>2015</risdate><volume>42</volume><issue>23</issue><spage>10,179</spage><epage>10,187</epage><pages>10,179-10,187</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>The Chang'E‐3 lunar penetrating radar (LPR) observations at 500 MHz reveal four major stratigraphic zones from the surface to a depth of ~20 m along the survey line: a layered reworked zone (&lt;1 m), an ejecta layer (~2–6 m), a paleoregolith layer (~4–11 m), and the underlying mare basalts. The reworked zone has two to five distinct layers and consists of surface regolith. The paleoregolith buried by the ejecta from a 500 m crater is relatively homogenous and contains only a few rocks. Population of buried rocks increases with depth to ~2 m at first, and then decreases with depth, representing a balance between initial deposition of the ejecta and later turnover of the regolith. Combining with the surface age, the LPR observations indicate a mean accumulation rate of about 5–10 m/Gyr for the surface regolith, which is at least 4–8 times larger than previous estimation. Key Points Chang'E‐3 high‐frequency lunar penetrating radar observations are presented Four major stratigraphic zones at the Chang'E‐3 landing site are observed Regolith accumulation rate is at least 4–8 times higher than previous estimation</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/2015GL066537</doi><tpages>9</tpages><oa>free_for_read</oa></addata></record>
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subjects Accumulation
Age
Basalt
Chinese spacecraft
Craters
Deposition
Depth
Ejecta
Ejection
Landing sites
Lunar exploration
Lunar landing
lunar penetrating radar
paleoregolith
Radar
Regolith
regolith thickness
Rock
Rocks
Stratigraphy
Surveying
title Regolith stratigraphy at the Chang'E-3 landing site as seen by lunar penetrating radar
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